To explore whether these correlations can be seen using light curve morphologies assigned
based on ZTF data, we cross-matched our variable star sample with photometry from
2MASS [1]}, WISE [2]}, [3]}, and Spitzer [4]}.
Figure REF  shows several color-color diagrams with the light curve morphologies
from Table REF  distinguished.
Figure REF  shows one infrared color as a function of our normalized variability amplitude metric.
Relative to the variability morphology vs infrared color analysis in [5]} studying Upper Sco and [6]} studying Taurus, we may be more subject here in the NAP region to the effects of reddening.
Thus, to de-redden the color-color diagrams, we adopted the \(A_V\)  values of in [7]}
and the near- and mid-infrared extinction results of [8]}.
Among our optical variables, about 78% have extinction values reported in [7]}.
For the remainder, we adopted the median value of \(A_V\) .
